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Long Wavelength Limit / Normal Modes Overview and Motivation Lecture 7 Phys 3750 Long Wavelength Limit / Normal Modes Overview and Motivation: Today we look at the long wavelength limit of the coupled-oscillator system. In this limit the equations of motion for the coupled oscillators can be transformed into the partial differential equation known as the wave equation, which has wide applicability beyond the coupled-oscillator system We also look at the normal modes and the dispersion relation for the coupled-oscillator system in this limit. Key Mathematics: We again utilize the Taylor-series expansion. I. Derivation of the Wave Equation A. The Long Wavelength Limit (LWL) So why look at the coupled-oscillator system at long wave lengths? Perhaps the main motivation comes from the fact that we are often interested in waves in systems where the wavelength is much longer than the distance between the coupled objects. For example, let's consider audible (ν = 20 to 20,000 Hz) sound waves in a solid. In a typical solid the speed of sound c is ~2000 m/s, so audible frequencies correspond to wavelengths ( λ = c ν ) between approximately 0.1 and 100 m. These wavelengths are obviously much greater that the typical interatomic spacing d of 2 × 10-10 m. As we will see, one benefit of the long wavelength limit is that we will no longer need to refer to the displacement of each interacting object: the index j will be "traded in" for the continuous position variable x , so that we will be considering displacements as a function of x and t . Let's consider the equation of motion for the j th oscillator (which can be any oscillator in the N coupled-oscillator system), d 2q ()t j = ω~2 []q ()t − 2q ()t + q ()t . (1) dt 2 j+1 j j−1 Let 's go ahead and trade in the discrete object index j for the continuous position variable x via x = jd , where d is the equilibrium distance between objects in the chain. Then we can rewrite Eq (1) as ∂ 2q()x,t = ω~ 2 []q()()()x + d,t − 2q x,t + q x − d,t . (2) ∂t 2 Notice that the time derivative is now a partial derivative because we are now thinking of the displacement q as a function of two continuous variables, x and t . D M Riffe -1- 1/10/2013 Lecture 7 Phys 3750 Now because d is a small parameter,1 let's Taylor series expand the two functions q()x + d,t and q()x − d,t in a Taylor series in d and − d , respectively, about the point x [so in doing this expansion we are thinking about x as some fixed point along the chain and q()x ± d,t as a function of ± d ]. The two Taylor series are ∂q()x,t 1 ∂ 2q(x,t) q()()x + d,t = q x,t + d + d 2 + (3a) ∂x 2 ∂x2 K and 2 ∂q()x,t 1 ∂ q(x,t) 2 q()()x − d,t = q x,t + ()− d + 2 ()− d +K (3b) ∂x 2 ∂x Keeping all terms up to order d 2 (we consider the validity of this approximation at the end of Sec. II) and substituting Eq. (3) into Eq. (2) gives us ∂ 2q()x,t ∂q 2 ()x,t = ω~ 2d 2 (4) ∂t 2 ∂x 2 This is the wave equation, which as you can see is a homogeneous, linear, second- order, partial differential equation. There is one more thing we need to do, however, in order to make Eq (4) more universally applicable. The term k ω~2d 2 = s d 2 (5) m on the rhs of Eq. (5) is a combination of the fundamental parameters ks , m , and d of 2 2 the coupled-oscillator problem. Let's define another constant c = ()ks m d so that we can more generically write the wave equation as ∂ 2q()x,t ∂q 2 ()x,t = c 2 . (6) ∂t 2 ∂x 2 1 Technically, the small parameter in the long wave length limit is the ratio d λ . Generally, a parameter can only be large or small if it is unitless. Otherwise, whether it is small or large (or somewhere in between) will depend upon the system of units being used. D M Riffe -2- 1/10/2013 Lecture 7 Phys 3750 B. General Applicability of the Wave Equation The is the standard form of the wave equation that we will use in this class. As we shall see in further study of the wave equation, c is the propagation speed of waves described by Eq. (6). Now if Eq. (6) were only useful for studying the long wavelength motion of the coupled-oscillator system, it really wouldn't be that interesting. Fortunately, it is applicable in a wide variety of situations, including sound waves in fluids and solids, transverse waves on a string, and electromagnetic waves in vacuum (or other nondispersive media). In each situation the constant c2 can be related to the underlying physics. For example, for transverse waves on a string, c2 = τ µ , where τ is the tension in the string and µ is the mass per unit length of the string. II. LWL of Coupled Oscillator Solutions A. Normal Modes Let's now look at the coupled-oscillator normal modes in the LWL. As we discussed in Lecture 6, we can write the normal-mode solutions (indexed by n ) as a function of x and t as iω()kn t −iω(kn )t q()n ()x,t = sin (kn x )()Ane + Bne (7) where the wave vector is given by nπ 1 k = , (8) n N +1 d and the dispersion relation is ~ d ω()kn = 2ω sin kn . (9) 2 As written, Eqs. (8) and (9) are expressed in terms of the fundamental (or microscopic) parameters d ,ω~ , and N of the coupled-oscillator problem. Let's see if we can re- express them in terms of c and other more generic (or macroscopic) parameters. Well, the first thing to notice is that the length L of the system (a more generic, macroscopic parameter) can be written in terms of the fundamental parameters N and d as L = ()N +1 d . The wave vector can thus be simply expressed as nπ k = . (10) n L D M Riffe -3- 1/10/2013 Lecture 7 Phys 3750 Well, what about Eq. (9), the dispersion relation? It is not yet clear what to do with ω~ in order to obtain a more generic description. This is where the long wavelength limit comes into play again. Recall that the wave vector is related to the wavelength via 2π kn = . (11) λn This allows us to write Eq. (9) as d ~ ω()λn = 2ω sinπ . (12) λn Now, the long wavelength limit is exactly the limit d λ << 1. Thus, in this limit we can replace the sine function by its (very small) argument, so that Eq. (12) can be expressed as ~ 2π ω()λn = ω d . (13) λn And now, using ω~ d = c and Eq (11), we have the long-wavelength-limit dispersion relation ω()kn = ckn . (14) Or, in a more general form that is applicable to any harmonic wave described by the wave equation (not just the normal modes for the coupled-oscillator system where k = kn is discrete), ω()k = ck . (15) So we see that, because c is constant, the dispersion relation for waves described by the wave equation is linear vs k . Looking back at the dispersion curves for the coupled-oscillator system that are plotted in the Lecture 6 notes, you should notice that for small kn k N (which is equivalent to small d λn ) that the dispersion curves are indeed linear vs kn . (The small wave vector limit is thus the same as the long wavelength limit.) Putting all of this together, we can write the normal modes [Eq. (7)] for long wavelengths as D M Riffe -4- 1/10/2013 Lecture 7 Phys 3750 nπ ic()nπ L t −ic()nπ L t q()n ()x,t = sin x()Ane + Bne (16) L A remark about the normal modes should be made at this point. The function sin()nπ x L in Eq. (16) came about because of the boundary conditions, which we can now express as q()0,t = 0 and q(L,t) = 0 [You can check that these boundary conditions are indeed satisfied by sin(nπ x L)]. For other boundary conditions we would generally get some linear combination of sin(kn x) and cos()kn x , and perhaps 2 also different allowed wave vectors kn (or equivalently, allowed wavelengths λn ). B. Neglect of Higher Order Terms in Equation of Motion in the LWL Now that we have an expression for the normal modes in the LWL, we can check to see that it is OK to neglect the terms in Eq. (3) that are of order higher than d 2 . The first thing to notice is that all the odd terms in Eqs. (3a) and (3b) cancel each other when inserted into Eq. (2). Thus we need only consider the even terms. The second thing to notice is that for even m m ∂mq ()x,t 2π ()n = −1 m 2 q x,t m () ()n (). (17) ∂x λn {This is obtainable using Eq. (16) in Eq. (3) [in Eq. (2)]}. Therefore, for example, the ratio of the 4th order term to the 2nd order term, neglecting numerical factors, is given by d 2 λ2 , which is much smaller than 1.
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